Temporal evolutions of the solar wind conditions at 1 AU prior to the near‐Earth X lines in the tail: Superposed epoch analysis

Author:

Zhang L. Q.1,Dai L.1,Baumjohann W.2,Lui A. T. Y.3,Wang C.1,Rème H.45,Dunlop M. W.67ORCID

Affiliation:

1. State Key Laboratory of Space WeatherNational Space Science Center, Chinese Academy of Sciences Beijing China

2. Space Research InstituteAustrian Academy of Sciences Graz Austria

3. Applied Physics LaboratoryThe Johns Hopkins University Laurel Maryland USA

4. University of Toulouse, UPS‐OMP, IRAP Toulouse France

5. CNRS, IRAP, BP 44346, F‐31028 Toulouse France

6. Space Research Institute, School of AstronauticsBeihang University Beijing China

7. Space Sciences DivisionRutherford Appleton Laboratory Didcot UK

Funder

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Cited by 5 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Anisotropic Vorticity Within Bursty Bulk Flow Turbulence;Journal of Geophysical Research: Space Physics;2020-10

2. BBF Deceleration Down‐Tail of X < −15 R E From MMS Observation;Journal of Geophysical Research: Space Physics;2020-02

3. Study on the vorticity field within the tail reconnection jet by the MMS spacecraft;2020-01-26

4. Measurements of the Vorticity in the Bursty Bulk Flows;Geophysical Research Letters;2019-09

5. Magnetospheric Physics in China;Chinese Journal of Space Science;2018

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